Table 2.
Spectroscopic, sample-selection, and structural characteristics of the INSPIRE DR1 sample.
ID | Sample | zXSH | zprev | M⋆ | ⟨Re⟩ | ⟨Re⟩ | Re, r | Re, r | nr | qr | R50UVB | R50VIS |
---|---|---|---|---|---|---|---|---|---|---|---|---|
KiDS | (1011 M⊙) | (″) | (kpc) | (″) | (kpc) | (″) | (″) | |||||
J0211–3155 | T18 | 0.3012 | 0.30135 | 0.876 | 0.237 | 1.07 | 0.237 | 1.07 | 8.1 | 0.48 | 0.58 | 0.55 |
J0224–3143 | T18 | 0.3839 | 0.3853 | 2.710 | 0.292 | 1.55 | 0.247 | 1.31 | 6.1 | 0.39 | 0.55 | 0.55 |
J0226–3158 | T18 | 0.2355 | 0.2364 | 0.688 | 0.350 | 1.32 | 0.337 | 1.27 | 3.7 | 0.60 | 0.58 | 0.50 |
J0240–3141 | T18 | 0.2789 | 0.2809 | 0.981 | 0.189 | 0.81 | 0.189 | 0.81 | 8.1 | 0.27 | 0.60 | 0.50 |
J0314–3215 | T18 | 0.2874 | 0.2888 | 1.000 | 0.150 | 0.66 | 0.148 | 0.65 | 5.5 | 0.39 | 0.55 | 0.50 |
J0316–2953 | T18 | 0.3596 | 0.3102 | 0.873 | 0.200 | 1.02 | 0.200 | 1.02 | 3.5 | 0.31 | 0.58 | 0.50 |
J0317–2957 | T18 | 0.2611 | 0.2610 | 0.873 | 0.257 | 1.05 | 0.257 | 1.05 | 5.0 | 0.21 | 0.59 | 0.50 |
J0321–3213 | T18 | 0.2947 | 0.2953 | 1.233 | 0.309 | 1.37 | 0.281 | 1.25 | 4.9 | 0.39 | 0.60 | 0.50 |
J0326–3303 | T18 | 0.2971 | 0.2976 | 0.930 | 0.321 | 1.44 | 0.321 | 1.44 | 3.7 | 0.35 | 0.60 | 0.50 |
J0838+0052 | S20 | 0.2702 | 0.2703 | 0.870 | 0.306 | 1.28 | 0.351 | 1.47 | 4.0 | 0.41 | 0.55 | 0.50 |
J0842+0059 | S20 | 0.2959 | 0.2946 | 0.910 | 0.226 | 1.01 | 0.226 | 1.01 | 3.3 | 0.29 | 0.55 | 0.50 |
J0847+0112 (*) | T18 | 0.1764 | 0.17636 | 0.989 | 0.456 | 1.37 | 0.465 | 1.40 | 3.3 | 0.26 | 0.60 | 0.55 |
J0857–0108 | S20 | 0.2694 | 0.2696 | 1.000 | 0.336 | 1.40 | 0.366 | 1.53 | 2.9 | 0.33 | 0.60 | 0.55 |
J0918+0122 | T18 | 0.3731 | 0.3733 | 2.263 | 0.328 | 1.71 | 0.328 | 1.71 | 6.0 | 0.51 | 0.60 | 0.55 |
J0920+0212 (*) | T18 | 0.2800 | 0.2797 | 1.031 | 0.345 | 1.48 | 0.345 | 1.48 | 2.0 | 0.32 | 0.58 | 0.55 |
J2305–3436 | T18 | 0.2978 | 0.30146 | 0.857 | 0.307 | 1.29 | 0.293 | 1.23 | 3.4 | 0.40 | 0.55 | 0.50 |
J2312–3438 | T18 | 0.3665 | 0.3664 | 1.344 | 0.243 | 1.25 | 0.243 | 1.25 | 2.3 | 0.43 | 0.60 | 0.60 |
J2327–3312 | T18 | 0.4065 | 0.40661 | 1.569 | 0.276 | 1.15 | 0.276 | 1.51 | 5.9 | 0.67 | 0.58 | 0.50 |
J2359–3320 | T18 | 0.2885 | 0.28922 | 1.065 | 0.237 | 1.03 | 0.237 | 1.04 | 4.4 | 0.39 | 0.58 | 0.50 |
Notes. In the first block of columns, we provide the KiDS publication from where each candidate was taken and the new redshifts inferred from XSH spectra. The first column of the second block lists instead the previously estimated redshifts. The two values are always in fair agreement. The previous redshifts, as well as the median (gri) size and stellar masses also provided in the same block, have been used for the INSPIRE object selection. The third block lists the structural parameters presented in T18 and/or S20 and obtained from the r-band KiDS images (the image with the best seeing), which are also shown in the histograms in Fig. 3, together with stellar masses. Finally, in the last block of columns, we report the apertures that encapsulate 50% of the light for the UVB and VIS arm, respectively (see Sect. 4.1). (*)Also observed in GAMA.
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